We use the high-resolution TNG50 cosmological magnetohydrodynamical simulation to
explore the properties and origin of cold circumgalactic medium (CGM) gas around massive …

Multi-phase filamentary structures around brightest cluster galaxies (BCG) are likely a key
step of AGN-feedback. We observed molecular gas in three cool cluster cores, namely …

We present an analysis of new and archival ALMA observations of molecular gas in 12
central cluster galaxies. We examine emerging trends in molecular filament morphology and …

Abstract We present Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 5 and
Cycle 6 observations of CO (2− 1) and CO (3− 2) emission at 0 farcs 2− 0 farcs 3 resolution …

To advance our understanding of the fuelling and feedback processes which power the
Universe's most massive black holes, we require a significant increase in our knowledge of …

We present observations using the Atacama Large Millimeter/submillimeter Array of the CO
(2− 1), HCN (3− 2), and HCO+(3− 2) lines in the nearby radio galaxy/brightest cluster galaxy …

Galaxies often contain large reservoirs of molecular gas that shape their evolution. This can
be through cooling of the gas–which leads to star formation, or accretion on to the central …

The origin of the cold gas in central galaxies in groups is still a matter of debate. We present
Multi-Unit Spectroscopic Explorer (MUSE) observations of 18 optically selected local (z≤ …

We present a study of molecular gas, traced via CO (3–2) from Atacama Large Millimeter/
submillimeter Array data, of four z< 0.2,'radio quiet', type 2 quasars (Lbol∼ 1045.3–1046.2 …

We present new Karl G. Jansky Very Large Array (JVLA) and Very Long Baseline Array
(VLBA) observations that traced the HI in the central region of 3C 84 (Perseus A). This radio …